Compressibility effect during the development of the tearing instability in a nonneutral current sheet in the solar atmosphere

Details Compressibility effect during the development of the tearing instability in a nonneutral current sheet in the solar atmosphere Compressibility effect during the development of the tearing instability in a nonneutral current sheet in the solar atmosphere

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..556v&link_type=abstract

Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 70, no. 3, p. 556-562.

Other

Compressibility Effects, Current Sheets, Magnetic Field Reconnection, Magnetohydrodynamic Stability, Solar Atmosphere, Solar Flares, Tearing Modes (Plasmas)

Scientific paper

It is shown that plasma compressibility stimulates the development of the tearing instability of a reconnecting current sheet in the LW region, where instability is absent in the approximation of an incompressible plasma. The longitudinal magnetic field plays the role of a trigger in this destabilization process, which is crucial to the physics of flares and other variable phenomena in the solar atmosphere.

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